scholarly journals Towards the solution of the relativistic gravitational radiation reaction problem for binary black holes

2001 ◽  
Vol 18 (19) ◽  
pp. 3989-3994 ◽  
Author(s):  
Carlos O Lousto
Keyword(s):  
Black Holes ◽  
Gravitational Radiation ◽  
Radiation Reaction ◽  
Binary Black Holes ◽  
Reaction Problem ◽  
Radiation Reaction Problem

Modeling gravitational radiation from coalescing binary black holes

2002 ◽  
Vol 65 (12) ◽  
Author(s):  
J. Baker ◽  
M. Campanelli ◽  
C. O. Lousto ◽  
R. Takahashi
Keyword(s):  
Black Holes ◽  
Gravitational Radiation ◽  
Binary Black Holes

scholarly journals Interpretations and Naturalness in the Radiation-Reaction Problem

Symmetry ◽  
2021 ◽  
Vol 13 (4) ◽  
pp. 658
Author(s):  
Carlos Barceló ◽  
Luis Garay ◽  
Jaime Redondo-Yuste
Keyword(s):  
Internal Structure ◽  
Equivalence Principle ◽  
Large Body ◽  
Radiation Reaction ◽  
Classical Electrodynamics ◽  
New Research ◽  
Reaction Problem ◽  
Radiation Reaction Problem

After more than a century of history, the radiation-reaction problem in classical electrodynamics still surprises and puzzles new generations of researchers. Here, we revise and explain some of the paradoxical issues that one faces when approaching the problem, mostly associated with regimes of uniform proper acceleration. The answers we provide can be found in the literature and are a synthesis of a large body of research. We only present them in a personal way that may help in their understanding. Besides, after the presentation of the standard answers, we motivate and present a twist to those ideas. The physics of emission of radiation by extended charges (charges with internal structure) might proceed in a surprising oscillating fashion. This hypothetical process could open up new research paths and a new take on the equivalence principle.

scholarly journals Binary black holes in Mkns as sources of gravitational radiation for space based interferometers

2003 ◽  
Vol 410 (2) ◽  
pp. 741-747 ◽  
Author(s):  
F. De Paolis ◽  
G. Ingrosso ◽  
A. A. Nucita ◽  
A. F. Zakharov
Keyword(s):  
Black Holes ◽  
Gravitational Radiation ◽  
Binary Black Holes

scholarly journals Binary-Single Encounters of 10 M⊙ Black Holes Including the Effects of Gravitational Radiation

1996 ◽  
Vol 174 ◽  
pp. 351-352
Author(s):  
K. N. Kong ◽  
H. M. Lee
Keyword(s):  
Black Holes ◽  
Gravitational Radiation ◽  
Stellar System ◽  
Radiation Reaction ◽  
High Mass ◽  
One Dimensional ◽  
Close Encounters ◽  
Dissipation Of Energy

We compute the outcomes of close encounters between a binary and a single black holes including the effects of gravitational radiation reaction. All masses of individual black holes are assumed to be 1 M⊙. We found that merger of two black holes takes place during the encounters in some cases. Thus the gravitational radiation can act as a mechanism for the dissipation of energy of a cluster mainly composed of 10 M⊙ black holes which are produced by the evolution of high mass stars. The merger probability depends on many parameters in a complex way. Our preliminary calculations show that about 10% of the strong encounters (i.e., rp ∼ a) between a binary of hardness 100 and a single lead to mergers of two black holes in the stellar system of one-dimensional velocity σ = 100 km/s.

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